The inclusive 56Fe(nu_e,e-)56Co cross section
arXiv:nucl-th/9905001 · doi:10.1103/PhysRevC.60.052801
Abstract
We study the 56Fe(nu_e,e^-)56Co cross section for the KARMEN neutrino spectrum. The Gamow-Teller contribution to the cross section is calculated within the shell model, while the forbidden transitions are evaluated within the continuum random phase approximation. We find a total cross section of 2.73 x 10^-40 cm^2, in agreement with the data.
4 pages, 1 figure. Replaced due to new improved calculations
Cited by in corpus (27)
- The Shell Model as Unified View of Nuclear Structure
- From eV to EeV: Neutrino Cross Sections Across Energy Scales
- Nuclear weak-interaction processes in stars
- Neutrino-nucleus reactions and nuclear structure
- The role of -induced reactions on lead and iron in neutrino detectors
- Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis
- Topical Review on "Beta-beams"
- What about a beta-beam facility for low energy neutrinos?
- Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random phase approximation
- Neutrino beams as a probe of the nuclear isospin and spin-isospin excitations
- Neutral-current neutrino-nucleus cross-sections for A~50-65 nuclei
- Neutrino-nucleus interaction rates at a low-energy beta-beam facility
- Neutrinos and nucleosynthesis of elements
- Nuclear Input for Core-collapse Models
- Neutrino and antineutrino charge-exchange reactions on 12C
- Detection of supernovae neutrinos with neutrino-iron scattering
- Uncertainties in modeling low-energy neutrino induced reactions on iron group nuclei
- Thermal effects on neutrino-nucleus inelastic scattering in stellar environments
- Forbidden transitions in neutral and charged current interactions between low-energy neutrinos and Argon
- Nuclear Weak Rates and Nuclear Weak Processes in Stars
- Lepton kinematics in low energy neutrino-Argon interactions
- Detecting supernova neutrinos with iron and lead detectors
- Low-energy neutrino scattering in experiment and astrophysics
- Inelastic nuclear scattering from neutrinos and dark matter
- QRAP: a numerical code for projected (Q)uasi-particle (RA)ndom (P)hase approximation
- Neutrino-nucleus interactions: open questions and future projects
- Supernova neutrino detection through neutron emission by nuclei